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Statistical variations of the elementary flux-pinning force and their effect on the shape of the bulk-pinning-force curve of high-field superconductors

Statistical variations of the elementary flux-pinning force and their effect on the shape of the... It is a common procedure to infer the flux-pinning mechanism from the shape of the bulk-pinning-force curve F p ( b ). In this paper, we investigate the effects of having a distribution of elementary pinning forces ( f p ) on F p ( b ) within the framework of fluxon core pinning and full summation. It is seen that the shape of F p ( b ) can be significantly changed when the pins are strong and their f p distribution broad, whereas traditional ideas accept that its shape remains constant. A shift of the peak of F p ( b ) to lower field and an increase in the curvature of the high-field portion of F p ( b ) is seen. We find confirmation of the model in optimized high- J c Nb-Ti composites, which have a broad distribution of α-Ti precipitate thicknesses. http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png Physical Review B American Physical Society (APS)

Statistical variations of the elementary flux-pinning force and their effect on the shape of the bulk-pinning-force curve of high-field superconductors

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Publisher
American Physical Society (APS)
Copyright
Copyright © 1992 The American Physical Society
ISSN
1095-3795
DOI
10.1103/PhysRevB.46.2964
Publisher site
See Article on Publisher Site

Abstract

It is a common procedure to infer the flux-pinning mechanism from the shape of the bulk-pinning-force curve F p ( b ). In this paper, we investigate the effects of having a distribution of elementary pinning forces ( f p ) on F p ( b ) within the framework of fluxon core pinning and full summation. It is seen that the shape of F p ( b ) can be significantly changed when the pins are strong and their f p distribution broad, whereas traditional ideas accept that its shape remains constant. A shift of the peak of F p ( b ) to lower field and an increase in the curvature of the high-field portion of F p ( b ) is seen. We find confirmation of the model in optimized high- J c Nb-Ti composites, which have a broad distribution of α-Ti precipitate thicknesses.

Journal

Physical Review BAmerican Physical Society (APS)

Published: Aug 1, 1992

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